The TESS photometry does not reveal any transits corresponding to the planets reported by [1]}.
If these planets are of Earth-like rocky composition, or have compositions similar to Solar System ice giants, their radii imply transit depths for edge-on orbits which exceed our detection thresholds. 1We conclude that either the planets are not in orbits that transit the host star, or that no transit of (Neptune-like) planets happened to occur during the TESS observation, or that (super-Earth) planets are smaller than models based on Solar System planets [2]} would predict.
